999精品在线视频,手机成人午夜在线视频,久久不卡国产精品无码,中日无码在线观看,成人av手机在线观看,日韩精品亚洲一区中文字幕,亚洲av无码人妻,四虎国产在线观看 ?

Post-solitons and electron vortices generated by femtosecond intense laser interacting with uniform near-critical-density plasmas

2022-04-12 03:44:38DongNingYue岳東寧MinChen陳民YaoZhao趙耀PanFeiGeng耿盼飛XiaoHuiYuan遠曉輝QuanLiDong董全力ZhengMingSheng盛政明andJieZhang張杰
Chinese Physics B 2022年4期

Dong-Ning Yue(岳東寧) Min Chen(陳民) Yao Zhao(趙耀) Pan-Fei Geng(耿盼飛)Xiao-Hui Yuan(遠曉輝) Quan-Li Dong(董全力) Zheng-Ming Sheng(盛政明) and Jie Zhang(張杰)

1School of Sciences,Harbin Institute of Technology at Weihai,Weihai 264209,China

2Key Laboratory for Laser Plasmas(Ministry of Education),School of Physics and Astronomy,Shanghai Jiao Tong University,Shanghai 200240,China

3Collaborative Innovation Center of IFSA,Shanghai Jiao Tong University,Shanghai 200240,China

4Key Laboratory of High Power Laser and Physics,Shanghai Institute of Optics and Fine Mechanics,Chinese Academy of Sciences,Shanghai 201800,China

5Tsung-Dao Lee Institute,Shanghai 200240,China

Keywords: stimulated Raman side scattering,near-critical-density plasmas,electron vortices,post-solitons

1. Introduction

The femtosecond intense laser plasma interaction has brought a number of applications such as laser-driven particle acceleration,[1-4]high-order harmonic generation,[5,6]postsolitons and electron vortices generation,[7-10]and so on.These applications depend on laser-plasma parameters such as plasma density,laser polarization,and so on. For underdense plasmas,laser-driven wakefields[1]are widely used to electron acceleration and the following compact radiation source.[2]For solid density plasmas,laser-driven ion acceleration is suggested as a potential way for future cancer therapyucite.[11,12]And high-order harmonic generation (i.e., laser-driven attosecond sources) can be applied in materials science and molecular biology.[6]For near-critical-density (NCD) plasmas,nonlinear physical processes or structures like stimulated Raman scattering (SRS),[13]post-solitons[7,14]and electron vortices[9,10,15,16]have also been studied.However,the symbiotic relationships of these structures have not been explored in detail.Since the NCD targets are unique to many applications,such as fast ignition,[17]strong magnetic field generation[18]and magnetic vortex ion acceleration,[19,20]it is necessary to explore the generation and evolution of such nonlinear structures,and their symbiotic relationships. On the other side,the recent processes on the supersonic gas jet[21,22]and foam target manufacture[23,24]make the NCD targets available in experiments.

In this paper, by using multi-dimensional particle-in-cell(PIC) simulations, we study the transportation of ultra-short intense laser pulse in NCD plasmas. It is found that the laser pulse undergoes strong stimulated Raman side scattering(SRSS) and transverse hosing instability. At the same time,nonlinear structures such as post-solitons and electron vortices are excited. The generation of these structures depends on the drive pulse polarization. To study these effects, we first use S-and P-polarized laser pulses in two-dimensional(2D)simulations. For the S-polarized drive case, the SRSS processes develop due to the relativistic effect and then the scattered waves evolve into post-solitons. Both the main laser pulse and scattered waves can drive electron convection currents forming electron vortices due to the Kelvin-Helmholtz instability(KHI).While for the P-polarized drive case, the SRSS waves deposit their energy into plasmas by heating surrounding electrons. Strong transverse currents resulting from the laser acceleration along the polarization direction are observed and electron vortices are formed. In the three-dimensional (3D)simulation,we have observed different structures in the planes along and perpendicular to the polarized direction of the laser pulse,which are consistent with the simulation observation in the two-dimensional simulations.

2. Strong SRSS process during ultra-short intense laser propagation in NCD plasmas

The relativistic PIC code OSIRIS[25]has been used to perform multi-dimensional simulations. A linearly polarized laser pulse with wavelength ofλ0=1.0μm propagates along thexdirection. The peak intensity of the laser isI0=5.0×1019W/cm2corresponding to a normalized laser electric field ofa0=6.0. The pulse takes Gaussian profiles both in longitudinal and transverse directions with a duration of 20.0 fs and FWHM focus size of 6.0 μm. The simulation boxes are 110 μm×30 μm for 2D and 40 μm×30 μm×30 μm for 3D simulations which are divided into 2200×600 and 640×480×480 cells,respectively. A plasma with uniform density 0.2ncis placed atx ≥0.0μm,wherenc=1.1×1021cm-3forλ0=1.0μm. The ion mass is set to bemi=3672.0me,wheremerepresents the rest mass of electron.

2.1. The S-polarization case

Strong SRSS process has been observed when the ultrashort intense laser pulse propagates in NCD plasmas. In Fig. 1(a) one can see that a strong SRSS wave is generated from the tail of the drive pulse. For the SRSS process, the three-wave matching conditions for the wave vector and frequency need to be satisfied,i.e.,

Fig.1. Distributions of laser electric field Ez in(a)spatial space(x,y)and(b)wave vector space(kx,ky)at t =20.0T0 for S-polarized laser case.(c) The temporal evolution of the normalized electric field Ez at point A in (a), where E0 =1.9×1013 V/m corresponding to a0 =6.0. (d) The SRSS frequency spectrum of Ez at point A in units of laser frequency ω0.

To analyze the SRSS process,we study the matching conditions and SRSS growth rate by considering the relativistic effects introduced by the drive laser. Distributions of the electric fieldEzin real space and in the wave vector space(kx,ky)are shown in Figs. 1(a) and 1(b). In Fig. 1(b), one can see that besides the main pulse, a strong SRSS wave with wave vector ofks=(0.62k,0.21k)appears att=20.0T0. The temporal evolution of this SRSS wave propagating through point A is shown in Fig.1(a). Its strength and spectrum are shown in Figs. 1(c) and 1(d). This SRSS wave is scattered by one of the plasma waves shown in Fig. 2(a). In Fig. 2(b), we show the corresponding wave vector of the plasma wave,i.e.,kp=(0.38k,-0.21k). The wavevector matching condition in Eq.(1)is satisfied for the three waves. A schematic view de-

For the SRSS waves, they are red-shifted and their frequencies go down when they propagate and dissipate energy.Eventually,they are captured by the surrounding plasmas and this results in the generation of post-solitons.[14]Such capture can happen outside of the plasma channel. We take the postsoliton in the dashed rectangle of Fig. 3(d) for an example.The post-soliton expands as a whole structure after the SRSS wave being captured which finally leaves an ion-bubble structure. With the post-soliton expanding, the frequency ofEzin it will be shifted to lower one[28]as shown in Fig.4(c).

Fig.2. Distributions of the longitudinal electric field Ex (i.e.,plasma waves)in(a)spatial space(x,y)and(b)wave vector space(kx,ky)at t =15.0T0.The schematics of SRSS physical process for an ultra-short intense laser pulse with(c)uniform intensity and(d)nonuniform intensity. Distributions of(e)electron density ne,(f)electron energy γe and(g)laser electric field Ez in spatial space(x,y)at t=15.0T0.

Fig. 3. Spatial distributions of (a) electric current vector and electron density ˉne, (b) magnetic field ˉBz, (c) longitudinal electric current density ˉJx at t=70.0T0 and(d)ion density ni at t=140.0T0. The solid and dashed black arrows in(c)represent the drive current and the return current,respectively.The red dashed rectangle in(d)represents one example of post-solitons which is formed by the captured SRSS wave.

Fig.4. (a)The temporal evolution of the transverse current density Jy at point B in Fig.3(a). (b)The temporal evolution of the laser electric field Ez in post-soliton marked by the red dashed rectangle in Fig.3(d). (c)The corresponding frequency spectrum of Ez in the post-soliton.

2.2. The P-polarization case

For the P-polarized laser case, we observe similar SRSS process shown in Figs. 5(a) and 5(b). However, unlike the formation of post-solitons in the S-polarized case, the SRSS waves dissipate their energy quickly by heating electrons. As we show in Figs.5(c),6(b),and 6(d),the electrons around the main pulse are severely disturbed by the SRSS waves. Electrons can be repelled by the ponderomotive force of the main pulse to form an electron bubble as one can see in Figs. 6(b)and 6(d). The front of the electron bubble severely interacts with the main pulse and oscillates along the opposite of the polarized direction as one can see in Fig. 6. Such oscillation frequencyωLis proportional to the plasma density,[10]i.e.,ωL≈ω2p/ω0≈0.2ω0. As shown in Figs. 6(a) and 6(b),the laser pulse hoses downward which causes the charge separation field to deflect downward as marked by the blue arrow att=25.0T0. While att=28.0T0, the laser pulse hoses upward and causes the charge separation field to deflect upward as given in Figs. 6(c) and 6(d). Such hosing oscillation finally results in the production of a wave-like plasma channel as shown in Fig. 7(d). The oscillation amplitude is so large that the bubble deviates from the laser axis.

The hosing oscillation process also generates strong transverse currents on the two sides of the plasma channel.The couple between these adjacent transverse currents results in the two rows of electron vortices and associated magnetic islands as shown in Figs.7(a)and 7(b). The strong convective currents driven by the P-polarized pulse are also observed in Fig. 7(c). As one can see. the KH-type structures are found outside of the plasma channel which indicates that KHI may also play a role for the generation of such electron vortices.

Fig.5. Distributions of laser electric field Ey in(a)spatial space(x,y)and(b)wave vector space(kx,ky)at t=20.0T0 for P-polarized case. (c)The distribution of electron density ne in spatial space(x,y)at t=20.0T0.

Fig. 6. The distributions of (a), (c) laser electric field Ey and (b), (d) electron density ne in spatial space (x,y) at (a), (b) t =25.0T0 and (b),(d)t=28.0T0. The blue arrows in(b)and(d)represent the transverse oscillating direction.

Fig. 7. Spatial distributions of (a) electron density ˉne, (b) magnetic field ˉBz, (c) longitudinal electric current density ˉJx and (d) ion density ni at t=70.0T0.

3. Wave-like plasma channel, SRSS wave and electron vortices in 3D geometry

To further confirm the SRSS process and the generation of KH-type electron vortices in an ultra-short laser near-criticaldensity plasma interaction,we have performed a 3DPIC simulation. The laser pulse is linearly polarized along theydirection. The simulation results are given in Fig. 8. As one can see from Figs. 8(a) and 8(c), after the laser pulse leaves,a plasma channel with central current filament is left. Such current filament has been investigated for magnetic dipole vortex ion acceleration.[29]Associated with the current filament,magnetic dipole vortex vectors are plotted by the red cones in Fig. 8(a). In thexyplane (P-polarized plane), we observe a wave-like plasma channel caused by hosing oscillation,which is related to the polarization of the drive pulse. We also observe side channels driven by SRSS waves in thexzplane(Spolarized plane)as shown in Fig.8(b). Besides,compared to 2D geometry,the return current strength is generally weak due to dimensional effects as shown in Fig.8(c). However,the unstable condition of KHI can also be satisfied as long as the single shear flow is strong enough when the return current is negligible, i.e.,Γ2KHI=(kh·V1)2>0. We can also observe the KH-type electron vortices induced by the KHI. Magnetic field associated with electron vortices, i.e., magnetic-islands structure,and one example of vortical current vector are plotted in Figs. 8(d) and 8(e), respectively. However, since the central axial current in the filament is so strong that it is hard to observe electron vortices induced by the hosing oscillation of the laser pulse. These characteristics are corresponding to the polarized planes as we found in 2D geometry.

Fig. 8. (a) Spatial distribution of 3D plasma channel. Both xy and xz planes are cut right through the channel central axis, while the yz plane is corresponding to the slice at x=15.0 μm. Magnetic dipole vortex vectors are plotted by the red cones. Spatial distributions of (b) laser electric field Ey at t=30.0T0,(c)longitudinal current density Jx,(d)magnetic field By in xz plane at t=90.0T0. (e)Current vector of dashed red rectangle in(c)with electron density distribution as background at t=90.0T0. The linearly polarized drive pulse is polarized along the y direction.

4. Conclusion and perspectives

In conclusion, we have studied the transportation of an ultra-short intense laser pulse and the nonlinear structures generation in near-critical-density plasmas. Nonlinear processes including SRSS process with relativistic effect and nonlinear structures generation,like electron vortices and post-solitons,are numerically studied. In 2D simulations, we analyze the evolution relationships of SRSS process,electron vortices and post-solitons with S-polarized and P-polarized laser pulses respectively. The laser pulses undergo similar SRSS processes generating scattering waves both for S-polarized and P-polarized cases. However,for the S-polarized case,the frequencies of SRSS waves drop down when the scattering waves further propagate in the plasma. These waves are eventually captured by the surrounding cold plasmas and result in the generation of post-solitons with ion bubbles. While for the P-polarized case, the SRSS waves quickly dissipate energy by heating electrons around the main pulse. The main pulse can drive convective electric currents forming electron vortices in the plasma channel for both cases. However, the mechanisms for the generation of electron vortices are different in the two cases. The KHI is the main mechanism for the S-polarized case, while for the P-polarized case, the hosing oscillation of the laser pulse plays an important role for electron vortices generation. We have also performed a 3DPIC simulation to further verify the existence of KH-type electron vortices. Wave-like structure in the polarized plane and side channel driven by SRSS waves are also observed. Our findings are helpful for future relative experimental studies.

Acknowledgments

The authors would like to acknowledge the OSIRIS Consortium, consisting of UCLA and IST (Lisbon, Portugal) for the use of OSIRIS and the visXD framework.Project supported by the National Natural Science Foundation of China (Grant Nos. 11991074, 11774227, 12005287,and 12135009), NSAF of China (Grant No. U1930111), the Natural Science Foundation of Shandong Province, China(Grant No. ZR2019ZD44), and the Strategic Priority Research Program of Chinese Academy of Sciences (Grant Nos.XDA25000000 and XDA25050800).

主站蜘蛛池模板: 亚洲福利一区二区三区| 自拍偷拍欧美| 亚洲男人天堂久久| 亚洲品质国产精品无码| 国产经典三级在线| 国产原创自拍不卡第一页| 91欧美在线| 中国一级毛片免费观看| 久久一日本道色综合久久| 亚洲经典在线中文字幕| 91九色国产在线| 欧美一级特黄aaaaaa在线看片| 久久久精品久久久久三级| 久久精品只有这里有| 欧美不卡视频在线观看| 国产无码网站在线观看| 国产区福利小视频在线观看尤物| 欧美色香蕉| 二级毛片免费观看全程| 九九免费观看全部免费视频| 波多野结衣一区二区三区四区| 亚洲欧美在线精品一区二区| 六月婷婷综合| 国产精品一区二区国产主播| 亚洲欧洲日本在线| 四虎永久在线精品影院| 国产成人福利在线| 国产在线一区二区视频| 日本在线国产| 中文字幕1区2区| 亚洲第一视频网| 免费播放毛片| 美女潮喷出白浆在线观看视频| 国产h视频免费观看| 日本成人精品视频| 国内自拍久第一页| 国产精品黄色片| 精品国产一区二区三区在线观看 | 欧美有码在线| 青青草原国产av福利网站| 亚洲精品成人片在线观看 | 九月婷婷亚洲综合在线| 小13箩利洗澡无码视频免费网站| 国产第三区| 国产门事件在线| 91啦中文字幕| 久久久久青草大香线综合精品| 国产福利在线免费| 国产在线97| 国产福利观看| 久久久噜噜噜久久中文字幕色伊伊 | 呦视频在线一区二区三区| 亚洲av色吊丝无码| 白浆免费视频国产精品视频| 亚洲精品第五页| 亚洲大尺码专区影院| 亚洲第一网站男人都懂| 国产无码在线调教| 成人综合在线观看| 色综合天天综合中文网| 九九热视频在线免费观看| 久久96热在精品国产高清| 亚洲天堂成人在线观看| 久久国产精品影院| 丰满人妻久久中文字幕| 亚洲中文字幕在线观看| 伊人久久大香线蕉aⅴ色| 91亚瑟视频| 亚洲国产精品日韩av专区| 国产欧美一区二区三区视频在线观看| 制服丝袜亚洲| 在线看片免费人成视久网下载| 制服丝袜亚洲| 一级毛片免费播放视频| 国内自拍久第一页| 2020精品极品国产色在线观看| 国产在线高清一级毛片| 欧美综合一区二区三区| 国产成人AV男人的天堂| 波多野吉衣一区二区三区av| 五月天综合网亚洲综合天堂网| 99久久精品免费看国产电影|